J/A+A/562/A106 Planck submillimetre sources in Virgo Cluster (Baes+, 2014)
The Herschel Virgo Cluster Survey.
XV. Planck submillimetre sources in the Virgo Cluster.
Baes M., Herranz D., Bianchi S., Ciesla L., Clemens M., De Zotti G.,
Allaert F., Auld R., Bendo G.J., Boquien M., Boselli A., Clements D.L.,
Cortese L., Davies J.I., De Looze I., di Serego Alighieri S., Fritz J.,
Gentile G., Gonzalez-Nuevo J., Hughes T., Smith M.W.L., Verstappen J.,
Viaene S., Vlahakis C.
<Astron. Astrophys., 562, A106-106 (2014)>
=2014A&A...562A.106B 2014A&A...562A.106B
ADC_Keywords: Clusters, galaxy ; Galaxy catalogs; Photometry, infrared ;
Photometry, millimetric/submm
Keywords: galaxies: ISM - submillimeter: galaxies
Abstract:
We cross-correlate the Planck Catalogue of Compact Sources (PCCS) with
the fully sampled 84deg2 Herschel Virgo Cluster Survey (HeViCS)
fields. We search for and identify the 857 and 545GHz PCCS sources in
the HeViCS fields by studying their FIR/submm and optical
counterparts. We find 84 and 48 compact Planck sources in the HeViCS
fields at 857 and 545GHz, respectively. Almost all sources correspond
to individual bright Virgo Cluster galaxies. The vast majority of the
Planck detected galaxies are late-type spirals, with the Sc class
dominating the numbers, while early-type galaxies are virtually absent
from the sample, especially at 545GHz. We compare the HeViCS SPIRE
flux densities for the detected galaxies with the four different PCCS
flux density estimators and find an excellent correlation with the
aperture photometry flux densities, even at the highest flux density
levels. We find only seven PCCS sources in the HeViCS fields without a
nearby galaxy as obvious counterpart, and conclude that all of these
are dominated by Galactic cirrus features or are spurious detections.
No Planck sources in the HeViCS fields seem to be associated to
high-redshift proto-clusters of dusty galaxies or strongly lensed
submm sources. Finally, our study is the first empirical confirmation
of the simulation-based estimated completeness of the PCCS, and
provides a strong support of the internal PCCS validation procedure.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 99 84 857GHz PCCS sources in extended HeViCS survey area
table2.dat 99 48 545GHz PCCS sources in extended HeViCS survey area
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See also:
VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)
J/AJ/90/1681 : The Virgo Cluster Catalog (VCC) (Binggeli+, 1985)
J/MNRAS/419/3505 : The HeViCS Bright Galaxy Sample (Davies+, 2012)
J/MNRAS/428/1880 : Far-IR properties of VCC galaxies (Auld+, 2013)
J/A+A/552/A8 : 454 VCC galaxies revised coordinates
(di Serego Alighieri+, 2013)
J/A+A/574/A126 : HeViCS. XVIII. Star-forming dwarf galaxies (Grossi+, 2015)
Byte-by-byte Description of file: table1.dat table2.dat
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Bytes Format Units Label Explanations
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1- 5 A5 --- --- [PCCS1]
7- 9 I3 GHz Band [545/857] Planck band (545 or 857)
11- 23 A13 --- Name PCCS source name (GLLL.ll+BB.bb) (1)
25- 33 F9.5 deg RAdeg Right ascension (J2000)
35- 42 F8.5 deg DEdeg Declination (J2000)
44- 49 F6.3 Jy FPCCS Observed Planck flux density in Band (2)
51- 55 F5.3 Jy e_FPCCS rms uncertainty on FPCCS
57- 64 A8 --- Ctp Optical counterpart name
65 A1 --- --- [/]
66- 69 A4 --- Ctp2 Second optical counterpart name
71- 74 I4 --- VCC ? VCC (J/AJ/90/1681) name of first
optical counterpart
75 A1 --- --- [/]
76- 79 I4 --- VCC2 ? VCC (J/AJ/90/1681) name of second
optical counterpart
81- 86 A6 --- Type Morphological type (from the GOLDMine database)
88- 93 F6.3 Jy Sspire ? HeViCS SPIRE 350um (for table1, Band=857GHz)
or 500um (for table2, 545GHz) flux density (3)
95- 99 F5.3 Jy e_Sspire ? rms uncertainty on Sspire
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Note (1): Planck Catalogue of Compact Sources (PCCS) sources are identified as
PCCS1 857 GLLL.ll+BB.bb (table1) and PCCS1 545 GLLL.ll+BB.bb (table2)
(see Cat. VIII/91)
Note (2): the listed flux density is the standard DETFLUX estimate, see
Sect. 3.1 for details).
Note (3): For the sources with an identified counterpart. Details on how this
flux density has been obtained can be found in Sect. 3.1.
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History:
From electronic version of the journal
References:
Davies et al., Paper I 2010A&A...518L..48D 2010A&A...518L..48D
Cortese et al., Paper II 2010A&A...518L..49C 2010A&A...518L..49C
Clemens et al., Paper III 2010A&A...518L..50C 2010A&A...518L..50C
Smith et al., Paper IV 2010A&A...518L..51S 2010A&A...518L..51S
Grossi et al., Paper V 2010A&A...518L..52G 2010A&A...518L..52G
Baes et al., paper VI 2010A&A...518L..53B 2010A&A...518L..53B
de Looze et al., paper VII 2010A&A...518L..54D 2010A&A...518L..54D
Davies et al., Paper VIII 2012MNRAS.419.3505D 2012MNRAS.419.3505D, J/MNRAS/419/3505
Magrini et al., Paper IX 2011A&A...535A..13M 2011A&A...535A..13M
Corbelli et al., Paper X 2012A&A...542A..32C 2012A&A...542A..32C
Pappalardo et al., Paper XI 2012A&A...545A..75P 2012A&A...545A..75P
Auld et al., Paper XII 2013MNRAS.428.1880A 2013MNRAS.428.1880A, J/MNRAS/428/1880
di Serego Alighieri et al., Paper XIII 2013A&A...552A...8D 2013A&A...552A...8D, J/A+A/552/A8
de Looze et al., Paper XIV 2013MNRAS.436.1057D 2013MNRAS.436.1057D
Davies et al., Paper XVI 2014MNRAS.438.1922D 2014MNRAS.438.1922D
Pappalardo et al., Paper XVII 2015A&A...573A.129P 2015A&A...573A.129P, J/A+A/573/A129
Grossi et al., Paper XVIII 2015A&A...574A.126G 2015A&A...574A.126G, J/A+A/574/A126
(End) Patricia Vannier [CDS] 07-Apr-2014